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Steady Mass Loss Associated with Nova Outbursts*

Published online by Cambridge University Press:  12 April 2016

Mariko Kato
Mariko Kato*
Affiliation:
Department of Astronomy, Faculty of Science, University of Tokyo, Bunkyo-ku, Tokyo, Japan

Abstract

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The structure of optically thick mass-losing envelopes of white dwarfs are studied in relation to nova outbursts. A sequence of steady mass-loss solutions is constructed for a nova outburst from the maximum photospheric radius to the disappearance. Much of mass of the envelope will be blown out.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 80: Double Stars, Physical Properties and Generic Relations , 1984 , pp. 295 - 298
Copyright
Copyright © Reidel 1984

Footnotes

*

Paper presented at the Lembang-Bamberg IAU Colloquium No. 80 on ‘Double Stars: Physical Properties and Generic Relations', held at Bandung, Indonesia, 3-7 June, 1983.

References

Kato, M.: 1983a, Pubi. Astron. Soc. Japan 35, 33.Google Scholar
Kato, M.: 1983b, Pubi. Astron. Soc. Japan 35, in press.Google Scholar
Nariai, K. and Nomoto, K.: 1979, Proceedings of Fourth Annual Workshop on Dwarf Novae and Other Cataclysmic Variables, Rochester, p. 525.Google Scholar
Nariai, K., Nomoto, K., and Sugimoto, D.: 1980, Pubi. Astron. Soc. Japan 32, 473.Google Scholar
Ruggles, C. L. N. and Bath, G. T.: 1979, Astron. Astrophys. 80, 97.Google Scholar
Truran, J. W.: 1981, in Wilkinson, D. (ed.), Progress in Particle and Nuclear Physics, Vol. 6, Pergamon Press, Oxford. Google Scholar